JWST/CEERS sheds light on dusty star-forming galaxies: Forming bulges, lopsidedness, and outside-in quenching at cosmic noon

Open Access

Fig. 8.

Best SED models computed by CIGALE (Boquien et al. 2019) for the red core (red line), the blue disk (blue line), and the intermediate region (green line) of the DSFG ID15371 at z_spec = 1.921 (the same example galaxy shown in Figs. 5 and 7). We show in the legend the value of the reduced χ² ( $χ_{red}^{2}$ $\chi _{\mathrm{red}}^{2}$ ) for each SED fit. The dots are the flux measurements from HST/ACS and JWST/NIRCam.

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